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国家卫星气象中心
收稿日期:2009-01-20,
修回日期:2009-02-20,
网络出版日期:2009-12-25,
纸质出版日期:2009-12-25
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李元,戎志国,郑照军,刘京晶,张立军,张里阳,胡秀清,张勇,孙凌. 2008年FY-3A扫描辐射计可见近红外通道在轨场地定标[J]. 光学精密工程, 2009,17(12):2966-2974
Post Launch Site Calibration of the Visible and Near-Infrared Channels of FY-3A Visible and Infrared Radiometer in 2008[J]. Optics and precision engineering, 2009, 17(12): 2966-2974.
FY-3A扫描辐射计发射后的首次在轨场地定标试验于2008年9月在甘肃敦煌中国遥感卫星辐射校正场展开。通过使用ASD FR光谱仪测量场地地表反射比,使用CE318太阳光度计测量气溶胶光学厚度,使用敦煌国家气候观象台加放的探空观测计算水汽总量,获取了3天的有效试验数据。定标采用反射比基法并配合新的地表反射比修正算法开展:过境时刻地表反射比由陆表各向异性二向反射比模型算法计算得到,并使用实测的地表反射比数据进行修正;表观反射比通过6S模型计算并进行太阳天顶角余弦修正和日地距离修正。在非水汽吸收通道,计算得到的多天定标斜率稳定(相对标准差在2.6%以内),使用定标结果计算23种观测目标的表观反射比,与TERRA/MODIS相应通道结果一致。
After the launching of FY-3A in May
2008
calibrating the payload in orbit turned important. The first post launch site calibration experiment of FY-3A visible and infrared radiometer (VIRR) was held in 2008’s site calibration experiment in Dunhuang remote satellite radiometric calibration site
Gansu province
China. Because of the bidirectional reflectance anisotropies of the land surface
the precision of the visible and near-infrared channels’ post launch site calibration was disturbed obviously. Getting a correct directional reflectance through the observing view angle and at the right time payload passing over is an important work. The vertical reflectance of 11 synchronization points in Dunhuang site was measured by ASD FR spectral meter and standard reference board during the period 1 hour fore-and-aft the satellite passing over. With a new reflectance correction method the calibration precision was improved: the directional reflectance at the moment the platform passing by was calculated by the algorithm for modeling bidirectional reflectance anisotropies of the land surface (AMBRALS) invented by TERRA/MODIS land group and multiplied by the correction coefficients. The correction coefficients were gotten by dividing each vertical reflectance measured by ASD of 11 synchronization points by the one calculated by AMBRALS and averaging them. Results showed that in some bands
the difference between measured one and calculated one reached about 10%. It showed the efficiency and importance of the new correction method. The aerosol optical depth (AOD) was measured by 10 bands sun photometer CE318 placed near the synchronization region. The AOD of 550nm is calculated according to Junge distribution. The layer water content was calculated by the sounding data measured by Dunhuang national climatic station (No. 52418). The vapor pressure was calculated by the Wexler’s formulas. The apparent reflectance was calculated by the use of 6S model and was corrected by the sun zenith cosine and sun-earth distance. Totally 3 days’ (2008/09/06
2008/09/10
2008/09/11) calibration slopes and intercepts of FY-3A/VIRR were gotten. The relative standard deviation(RSD) of them was below 2.6%. In order to validating the post launch calibration’s veracity
23 targets’ apparent reflectances were compared by FY-3A/VIRR and TERRA/MODIS
they matched well. The results showed the stability and veracity of the calibration arithmetic except for the water vapor absorption bands. In vapor absorption bands
the 3 days’ slopes varied obviously. Compared to the pre launch calibration
the post launch calibration changed about 7.73%~21.52% in different bands
showed the imperative of post launch calibration right after the satellite launching. Now the pre launch calibration slopes and intercepts had been substituted by the post launch ones.
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